Efeito da radiação ionizante, simulando radioterapia, nas propriedades de cerâmicas Y-TZP e cimentos resinosos

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Utilização de material alternativo para a obtenção e caracterização de biomodelos, por meio da técnica de impressão 3DPRINTER

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Análises físico-químicas e biológicas de diferentes scaffolds à base de polihidroxibutirato e polihidroxibutirato-co-valerato

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Análises físico-químicas e biológicas de diferentes scaffolds à base de polihidroxibutirato e polihidroxibutirato-co-valerato

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Seleção de clones de figueira cv. roxo de Valinhos formados por gemas irradiadas

A figueira (Ficus carica L.), pertencente à família das Moráceas, constitui-se numa das mais importantes frutíferas cultivadas, elevando o Brasil à condição de décimo maior produtor e exportador de figos do mundo. Porém, a ficicultura apresenta alguns problemas fitossanitários, além de, no Brasil, estar toda implantada com uma única cultivar, a Roxo de Valinhos, que produz frutos sem sementes, inviabilizando o melhoramento convencional. Nesse sentido, o melhoramento genético, com o uso de mutagênicos, passa a ser uma linha de pesquisa altamente importante, podendo contribuir enormemente para o desenvolvimento da cultura. Diante disto, o objetivo do presente trabalho foi selecionar mutantes em plantas de figueira formadas por estacas irradiadas com raios gama, a fim de aumentar sua variabilidade genética com relação ao desenvolvimento vegetativo e reprodutivo. Utilizaram-se plantas formadas por estacas originadas de gemas da cultivar Roxo de Valinhos irradiadas com raios gama, no irradiador tipo Gamma a 0,10 m do ápice, na dose de Gy com taxa de dose de 238 Gy/h. O experimento constou de 450 tratamentos, sendo cada planta formada considerada um tratamento, numerando-as sequencialmente de 1 a 450 e cultivadas em espaçamento de 2,5 x 1,5 m.. As avaliações foram realizadas a partir das características tanto das folhas quanto dos frutos, bem como da incidência das principais pragas e doenças da cultura nestas plantas. Da análise dos dados, conclui-se que há variabilidade genética entre os tratamentos e que algumas plantas são prováveis mutantes, mostrando-se assim com potencial para posteriores estudos, devendo ser testadas em plantios comerciais.

Acúmulo de minerais em Aechmea blanchetiana (Baker) L.B. Smith (Bromeliaceae), contaminadas com zinco em cultivo in vitro

Com o objetivo de estudar a absorção e translocação de Ca, Co, Fe, K e Zn em Aechmea blanchetiana, plantas foram cultivadas in vitro em meios de cultivo contendo concentrações de Zn (0,0; 0,18; 1,8; 18 e 180 mg Zn L-1). Após 16 semanas de cultivo, os sistemas aéreo e radicular foram separados e determinadas à massa seca para massa de matéria seca e para a análise por ativação com nêutrons (AAN). O procedimento consistiu em irradiar amostras e padrões no reator nuclear de pesquisa IEA-R1 por 16 h para análise por espectrometria de raios gama. O controle dos resultados foi avaliado por meio das análises dos materiais de referência certificados, com desvios padrão relativo de 9,1 % e erros inferiores a 12,9 %. Os resultados das determinações dos elementos mostraram que o Zn alterou absorção e translocação de Ca, Co, Fe, K e Zn. A espécie apresentou alta quantidade de Zn nos sistemas aéreo e radicular indicando, possivelmente, ser bioacumuladora desse elemento.

Prospect on intergalactic magnetic field measurements with gamma-ray instruments

Observing high-energy gamma-rays from Active Galactic Nuclei (AGN) offers a unique potential to probe extremely tiny values of the intergalactic magnetic field (IGMF), a long standing question of astrophysics, astropa rticle physics and cosmology. Very high energy (VHE) photons from blazars propagating along the line of sight interact with the extragalactic background light (EBL) and produce e + e − pairs. Through inverse-Compton interaction, mainly on the cosmic microwave background (CMB), these pairs generate secondary GeV-TeV compo- nents accompanying the primary VHE signal. Such secondary components would be detected in the gamma-ray range as delayed “pair echos” for very weak IGMF ( B< 10 − 16 G ), while they should result in a spatially extended ga mma-ray emission around the source for higher IGMF values ( B> 10 − 16 G ). Coordinated observations with space (i.e. Fermi) and ground- based gamma-ray instruments, such as the pre sent Cherenkov experiments H.E.S.S., MAGIC and VERITAS, the future Cherenkov Telescope Array (CTA) Observatory, and the wide-field detectors such as HAWC and LHAASO, should allow to analyze and finally detect such echos, extended emission or pair halos, and to further characterize the IGMF.

Positron annihilation spectroscopy techniques applied to the study of an HPGe detector.

Doppler Broadening Spectroscopy of the large Ge crystal of an HPGe detector was perforrned using positrons from pair production of 6.13 MeV ϒ-rays from the 19F(p,αϒ) 16O reaction. Two HPGe detectors facing opposite sides of the Ge crystal acting as target provided both coincidence and singles spectra. Changes in the shape of the annihilation peak were observed when the high voltage applied to the target detector was switched on or off, amounting to somewhat less than 20% when the areas of equivalent energy intervals in the corresponding normalized spectra are compared.

Estudio acústico de la sala 8 de los cines Kinépolis de Ciudad de la Imagen

Este proyecto consistira en la realization de un estudio aciistico sobre la sala 8 de los cines Kinepolis de Ciudad de la Imagen, que dispone de 408 butacas. Los cines Kinepolis es uno de los mayores complejos multisala de Europa. Cuenta con mas de 9.200 butacas en total distribuidas en 25 salas a las que se accede mediante dos grandes pasillos conectados por el hall. En 1998, ano de su apertura, el complejo recibio el Record Guinness a la sala cinematografica mas grande del mundo, que dispone de 996 butacas. El objetivo de este proyecto es conseguir caracterizar acusticamente una sala de cine a traves de la medicion de parametros acusticos de la sala y de un modelo virtual de la misma. Para llevar a cabo el proyecto, primero se van a realizar tanto una medicion geometrica como acustica de la sala mediante el sistema de medida DIRAC. Los resultados de estas mediciones nos serviran para construir y validar un modelo virtual de la sala real con el software de simulacion EASE. La medicion acustica se va a realizar con el sistema de medicion DIRAC. Este sistema nos dara information sobre una amplia variedad de parametros acusticos. En este proyecto no se va a trabajar con todos ellos, solo con los mas significativos. Estos se describen a continuacion en la introduccion teorica. La medicion geometrica nos va a servir para construir un modelo virtual que tenga las mismas dimensiones que la sala original. Esta medicion la realizaremos mediante un medidor laser y una cinta metrica. Una vez construido el modelo virtual, se procedera a su validacion. Este proceso se realiza ajustando el tiempo de reverberacion del modelo mediante la introduccion de distintos materiales acusticos en las superficies del mismo, de manera que, variando la absorcion de la sala, el tiempo de reverberacion promedio del modelo se asemeje lo mas posible al medido en la sala real. Este proceso tiene como objetivo comprobar que el modelo virtual tiene un comportamiento acustico similar al de la sala real. Es necesario validar adecuadamente el modelo para que las comparaciones y conclusiones sean fiables. Por ultimo, tras la simulacion acustica del modelo, se compararan los resultados simulados con los medidos en la sala. En este proceso se contrastaran algunos de los parametros que guardan relation con el tiempo de reverberacion. De esta manera se verificara si el tiempo de reverberacion es o no un parametro acustico fiable para la validacion de un modelo virtual de una sala de cine. Anteriormente se han realizado proyectos iguales de otras salas de diferente tamano de Kinepolis. El objetivo de realizar el mismo estudio en distintas salas, es comprobar si el tamano de la sala influye en la validacion de los modelos virtuales mediante el tiempo de reverberacion. ABSTRACT. This Project consists on the development of an acoustic research of the movie theater 8 of the Kinepolis complex in Ciudad de la Imagen, Madrid. This room has 408 spots. Kinepolis is one of the biggest multiplex complexes in Europe. It has 9,200 locations disposed in 25 rooms. There are two large corridors which give access to all of theaters. In the middle of the structure, there is the main hall that connects these corridors. In 1998, at the time when the complex was open, it was awarded with the Record Guinness for the biggest theater in the world, which has 996 locations. The target of this project is to successfully characterize the acoustics of a movie theater through reverberation time and a virtual model. In order to reach this goal, in the first place, we are going to perform both, an acoustic and a geometric measurement of the room using DIRAC measurement system. The results of these measures will allow us to build and validate a virtual model of the room, using the simulation software EASE. We are going to use the DIRAC system in order to accomplish the acoustic measure. This operation gives us a huge variety of acoustic parameters. Not all of these are going to be used for this research, only the most significant ones. These are described in the theoretical introduction. The geometric measure is essential to help us to build the virtual model, because the model has to be exactly equal as the real room. This measurement will be performed with an electronic distance meter and a measuring tape. Once the virtual model is finished, it will be proved. This validation process will be realized by adjusting the reverberation time in the model. We will change the walls materials, therefore, the overall absorption of the room will change. We want the model reverberation time resemble to the real one. This practice is going to ensure that the model acoustic performance is close to the real one. In addition, it has to be successfully validate of we want the future comparisons to be reliable. Finally, after the model virtual simulation, we will compare the simulated results with the measure in the room. In this process, we will compare not only the reverberation time, but others parameters that keep relation with the reverberation time. We will verify this way, if the reverberation time is or is not an appropriate acoustic parameter to validate a virtual model of a movie theater. There have been done others similar acoustic researches in different theaters with different sizes. The aim of performing similar researches in different rooms is to determine if the size of the room infers in the validation process.

Análise espacial de reservatórios usando DFA de dados geofísicos

This research aims to set whether is possible to build spatial patterns over oil fields using DFA (Detrended Fluctuation Analysis) of the following well logs: sonic, density, porosity, resistivity and gamma ray. It was employed in the analysis a set of 54 well logs from the oil field of Campos dos Namorados, RJ, Brazil. To check for spatial correlation, it was employed the Mantel test between the matrix of geographic distance and the matrix of the difference of DFA exponents of the well logs. The null hypothesis assumes the absence of spatial structures that means no correlation between the matrix of Euclidean distance and the matrix of DFA differences. Our analysis indicate that the sonic (p=0.18) and the density (p=0.26) were the profiles that show tendency to correlation, or weak correlation. A complementary analysis using contour plot also has suggested that the sonic and the density are the most suitable with geophysical quantities for the construction of spatial structures corroborating the results of Mantel test

Análise wavelet da variabilidade do quasar 3C 273

Discovered in 1963, 3C 273 was the second quasar identified and cataloged in the Third Cambridge Catalog for radio sources, and the first one for which emission lines were identified with a hydrogen sequence redshifted. It is the brightest quasar of the celestial sphere, the most studied, analyzed, and with a resulting abundance of data available in a vast literature. The accurate analysis of the deviations of the spectral lines of quasars provides enough information to put in evidence the variation of fundamental constants of nature and similarly the universe expansion rate. The analysis of the variability of the light curves of these bodies, and the consequent accuracy of their periodicity, is of utmost importance as it provides an efficiency of their observations, enables a greater understanding of the physical phenomena, and makes it possible to conduct spectral observations on more accurate dates (when their light curves show pronounced peaks and therefore richer spectra information). In this master’s thesis twenty eight light curves from the quasar 3C 273 are studied, covering all the electromagnetic spectrum wavebands (radio emission to gamma rays), totaling in the analysis of four light curves for each waveband. We have applied the method of Continuous Wavelet Transform using the sixth-order (!0 = 6) Morlet wavelet function, and obtained excellent results in accordance with the literature.

Análise wavelet da variabilidade do quasar 3C 273

Discovered in 1963, 3C 273 was the second quasar identified and cataloged in the Third Cambridge Catalog for radio sources, and the first one for which emission lines were identified with a hydrogen sequence redshifted. It is the brightest quasar of the celestial sphere, the most studied, analyzed, and with a resulting abundance of data available in a vast literature. The accurate analysis of the deviations of the spectral lines of quasars provides enough information to put in evidence the variation of fundamental constants of nature and similarly the universe expansion rate. The analysis of the variability of the light curves of these bodies, and the consequent accuracy of their periodicity, is of utmost importance as it provides an efficiency of their observations, enables a greater understanding of the physical phenomena, and makes it possible to conduct spectral observations on more accurate dates (when their light curves show pronounced peaks and therefore richer spectra information). In this master’s thesis twenty eight light curves from the quasar 3C 273 are studied, covering all the electromagnetic spectrum wavebands (radio emission to gamma rays), totaling in the analysis of four light curves for each waveband. We have applied the method of Continuous Wavelet Transform using the sixth-order (!0 = 6) Morlet wavelet function, and obtained excellent results in accordance with the literature.

Desenvolvimento de protótipo de aplicativo móvel em Android® para o controle e acompanhamento nutricional da saúde óssea em mulheres menopáusicas

Following a drop in estrogen in the period of menopause some women begin to lose bone mass more than 1% per year reaching the end of five years with loss greater than 25%. In this regard, factors such as older age, low calcium intake and premature menopause favor the onset of osteoporosis. Preventive methods such as nutritional counseling to a proper diet and the support of technology through applications that assess dietary intake are essential. Thus, this study aimed to develop an application for Android® platform focused on the evaluation of nutritional and organic conditions involved in bone health and risks for developing osteoporosis in postmenopausal women. To achieve this goal we proceeded to a study of 72 women aged 46-79 years, from the physical exercise for bone health of the Laboratory for Research in Biochemistry and Densitometry the Federal Technological University of Paraná program. Data were collected in the second half of 2014 through tests Bone Densitometry and Body Composition, Blood Tests, Anthropometric data and Nutrition Assessment. The study included women with a current diagnosis of osteopenia or osteoporosis primary, aged more than 45 years postmenopausal. For the assessment of bone mineral density and body composition used the device Absorptiometry Dual Energy X-ray (DXA) brand Hologic Discovery TM Model A. For anthropometric assessment was included to body mass, height, abdominal circumference, Waist circumference and hip circumference. The instrument for assessing food consumption was used Recall 24 hours a day (24HR). The estimated intake of energy and nutrients was carried from the tabulation of the food eaten in the Software Diet Pro 4®. In a sub sample of 30 women with osteopenia / osteoporosis serum calcium and alkaline phosphatase tests were performed. The results demonstrated a group of women (n = 30) average calcium intake of 570mg / day (± 340). The analysis showed a mean serum calcium within the normal range (10,20mg / dl ± 0.32) and average values and slightly increased alkaline phosphatase (105.40 U / L ± 23.70). Furthermore, there was a significant correlation between the consumption of protein and the optimal daily intake of calcium (0.375 p-value 0.05). Based on these findings, we developed an application early stage in Android® platform operating system Google®, being called OsteoNutri. We chose to use Java Eclipse® where it was executed Android® version of the project; choice of application icons and setting the visual editor for building the application layouts. The DroidDraw® was used for development of the three application GUIs. For practical tests we used a cell compatible with the version that was created (4.4 or higher). The prototype was developed in conjunction with the Group and Instrumentation Applications Development (GDAI) of the Federal Technological University of Paraná. So this application can be considered an important tool in dietary control, allowing closer control consumption of calcium and dietary proteins.

Desenvolvimento de formulações para produção de grés porcelanato a partir de matérias-primas da região da bacia do Parnaíba

Brazil is a great ceramic raw materials productor because of the its big number of clay deposits, in various areas of the ceramic industry. Although, the majority of the natural reservations are unknown or not studied yet, so there is no scientific technical dates that can guide their usage and industrial application, as well as the racional and optimazed way of usage by the industrial sector. The state of Maranhão has a gigant mineral wealth as esmectite, bentonite, kaolin, clays, feldspates, marine salt, iron and others, but produce only products with small agregated value compared to the porcelanato, one of the most expensives ceramic cover tiles, the reason for that is the low water absorption (lower than 0,5%), beside present amazing tecnicals features, like mechanical resistence. The main objective of the work is to do the characterization of four clays, with the finallity of find an application by the results and develop formulations to produce porcelanato using these raw materials from Timon-MA. For this were made the raw materials characterization using X ray fluorecence; X ray diffraction; Differencial thermal analysis; Dilatometric analysis and Tecnological properties, planing three formulations that were sinterized at six different temperatures: 1150, 1170, 1190, 1210, 1230 and 1250ºC for 7 minutes. After the sinteratization, the samples were submitted to tension resistance analysis. Were attained two formulations with the requested properties to produce porcelanato

Correlações nos dfa de diversos perfis geológicos. estudo de caso: Bacia de Campos - RJ

This work aims to study the fluctuation structure of physical properties of oil well profiles. It was used as technique the analysis of fluctuations without trend (Detrended Fluctuation Analysis - DFA). It has been made part of the study 54 oil wells in the Campo de Namorado located in the Campos Basin in Rio de Janeiro. We studied five sections, namely: sonic, density, porosity, resistivity and gamma rays. For most of the profiles , DFA analysis was available in the literature, though the sonic perfile was estimated with the aid of a standard algorithm. The comparison between the exponents of DFA of the five profiles was performed using linear correlation of variables, so we had 10 comparisons of profiles. Our null hypothesis is that the values of DFA for the various physical properties are independent. The main result indicates that no refutation of the null hypothesis. That is, the fluctuations observed by DFA in the profiles do not have a universal character, that is, in general the quantities display a floating structure of their own. From the ten correlations studied only the profiles of density and sonic one showed a significant correlation (p> 0.05). Finally these results indicate that one should use the data from DFA with caution, because, in general, based on geological analysis DFA different profiles can lead to disparate conclusions